Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …

When discussing research in physics and in science more generally, it is common to ascribe
equal importance to the three components of the scientific trinity: theoretical, experimental …

The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed
largely in the early 1990s, together with an important extension to inhomogeneous flows in …

A comprehensive overview is presented of recent observational and theoretical results on
solar wind structures and fluctuations and magnetohydrodynamic waves and turbulence …

We present experimental and theoretical evidence suggesting that the mean free path of
cosmic-ray electrons and protons may be fundamentally different at low to intermediate (less …

We present a series of models for the plasma properties along open magnetic flux tubes
rooted in solar coronal holes, streamers, and active regions. These models represent the …

Abstract The Parker Solar Probe (PSP) entered a region of sub-Alfvénic solar wind during
encounter 8, and we present the first detailed analysis of low-frequency turbulence …

The 2D+ slab superposition model of solar wind turbulence has its theoretical foundations in
nearly incompressible magnetohydrodynamics (NI MHD) in the plasma beta∼ 1 or≪ 1 …

The complex nonlinear dynamical phenomenon described as turbulence, is known to have
a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper …

In a previous paper we argued that the dam** of obliquely propagating kinetic Alfvén
waves, chiefly by resonant mechanisms, was a likely explanation for the formation of the …